Zobrazeno 1 - 10
of 15
pro vyhledávání: '"L. V. Tóth"'
Context. Studies of the interstellar medium and the pre-stellar cloud evolution require spectral line observations that have a high sensitivity and high angular and velocity resolution. Regions of high-mass star formation are particularly challenging
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9571b61eb5825f0ba39564b5a4a109c5
http://hdl.handle.net/10138/351285
http://hdl.handle.net/10138/351285
Autor:
R. Bőgner, T. Csengeri, J. Montillaud, M. Wienen, N. Schneider, F. Wyrowski, F. Motte, L. V. Tóth
Publikováno v:
Astronomy & Astrophysics. 667:A137
Context. The Rosette molecular cloud complex is a well-known Galactic star-forming region with a morphology pointing towards triggered star formation. The distribution of its young stellar population and the gas properties point to the possibility th
Publikováno v:
Origins: From the Protosun to the First Steps of Life. Proceedings of the International Astronomical Union
Origins: From the Protosun to the First Steps of Life. Proceedings of the International Astronomical Union, Aug 2018, Vienna, Austria. pp.371-372, ⟨10.1017/S1743921319002254⟩
Origins: From the Protosun to the First Steps of Life. Proceedings of the International Astronomical Union, Aug 2018, Vienna, Austria. pp.371-372, ⟨10.1017/S1743921319002254⟩
Recent theories on the formation of the Solar System turned the attention to the study of low mass cloud cores in massive star forming regions. The Rosette Molecular Cloud is a well-known star forming area having highly filamentary structure with den
Autor:
Munetaka Ueno, Yoshimi Kitamura, L. V. Tóth, Gábor Marton, Motohide Tamura, Sarolta Zahorecz, Akiko Kawamura
Publikováno v:
Astronomische Nachrichten. 334:928-931
Large area surveys allow us to identify young stellar objects and classify them based on their colours. The near-, mid- and far-infrared filters' sensitivities are different, therefore different proportions of young stars are observable. Evolutionary
Autor:
Roberta Paladini, D. J. Marshall, L. Montier, J. Montillaud, I. Ristorcelli, J. Malinen, P. M. McGehee, C. Lefèvre, Nathalie Ysard, Peter G. Martin, V.-M. Pelkonen, A. Rivera-Ingraham, L. V. Tóth, Mika Juvela, J.-P. Bernard, Laurent Pagani
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2015, 584, pp.A93. ⟨10.1051/0004-6361/201423788⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2015, 584, pp.A93. ⟨10.1051/0004-6361/201423788⟩
Astronomy and Astrophysics-A&A, 2015, 584, pp.A93. ⟨10.1051/0004-6361/201423788⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2015, 584, pp.A93. ⟨10.1051/0004-6361/201423788⟩
The project Galactic Cold Cores has made Herschel observations of interstellar clouds where the Planck satellite survey has located cold and compact clumps. The sources range from starless clumps to protostellar cores. We examine 116 Herschel fields
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::26df1fb369b3455823eeaf02e24bcae4
https://cea.hal.science/cea-01383764
https://cea.hal.science/cea-01383764
Publikováno v:
Proceedings of the International Astronomical Union. 12:166-167
One of the most certain ways to determine star formation rate in galaxies is based on far infrared (FIR) measurements. To decide the origin of the observed FIR emission, subtracting the Galactic foreground is a crucial step. We utilized Herschel phot
Autor:
Gábor Marton, Annie Zavagno, Frédérique Motte, P. M. McGehee, Laurent Pagani, I. Ristorcelli, D. J. Marshall, Mika Juvela, Nathalie Ysard, V.-M. Pelkonen, L. V. Tóth, J.-P. Bernard, Sarolta Zahorecz, J. Malinen, Roberta Paladini, E. Falgarone, L. Montier, J. Montillaud, A. Rivera-Ingraham, Yasuo Doi
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2015, 584, pp.A92. ⟨10.1051/0004-6361/201424063⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2015, 584, pp.A92. ⟨10.1051/0004-6361/201424063⟩
Astronomy and Astrophysics-A&A, 2015, 584, pp.A92. ⟨10.1051/0004-6361/201424063⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2015, 584, pp.A92. ⟨10.1051/0004-6361/201424063⟩
Context. For the project Galactic cold cores, Herschel photometric observations were carried out as a follow-up of cold regions of interstellar clouds previously identified with the Planck satellite. The aim of the project is to derive the physical p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::20eaa346ee9977ef8ca9220dfab44f5c
https://hal.science/hal-01277975/document
https://hal.science/hal-01277975/document
Publikováno v:
Astronomy & Astrophysics. 456:1037-1043
Aims. The purpose of this study is to investigate the distributions of the isomeric molecules HCN and HNC and estimate their abundance ratio in the protostellar core Cha-MMS1 located in Chamaeleon {\sc i}. Methods. The core was mapped in the J=1-0 ro
Publikováno v:
Astronomy & Astrophysics. 453:923-936
Aims. A complex study of visual and infrared properties of ISM and an examination of cloud morphology was carried out using USNO, 2MASS, DIRBE, IRAS, and ISO data of an extended region in Cepheus to explore the conditions of cloud and star formation.
Publikováno v:
Astronomy & Astrophysics. 420:533-546
Three prominent cold objects of the Taurus Molecular Ring (TMR) were revealed by our ISOPHOT 200 µ mm ap of the south-eastern part of the Heiles Cloud 2 (HCL 2) cloud complex. One corresponds to the cyanopolyyne peak region of the TMC-1 ridge, (TMC-